Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
96.8668 -20.0413 0.0156 4.6735 -40.1182 1.2491770 12.276 TRIG_01205899
Foreground time interval of the image:
7.832 72.701 (delta_t = 64.869 [sec])
Background time interval of the image:
-239.000 7.832 (delta_t = 246.832 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
- 4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
- 5) Time of each bin is in the middle of the bin.
1 s binning
From T0-310 s to T0+310 s
From T100_start - 20 s to T100_end + 30 s
Full time interval
64 ms binning
Full time interval
From T100_start to T100_end
From T0-5 sec to T0+5 sec
16 ms binning
From T100_start-5 s to T100_start+5 s
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
- 3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from 7.832 sec. to 133.496 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98196 ( -0.217865 0.233332 )
Norm@50keV : 7.02250E-04 ( -0.000112606 0.000109951 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.10 using 59 bins.
Reduced chi-squared = 1.08947
# Null hypothesis probability of 3.00e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 125.7 sec: 0.104481 ( -0.0127102 0.012709 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.13478e-07 ( -1.21941e-07 1.25349e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.832 sec. to 133.496 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.881953 ( -1.23367 1.00584 )
Epeak [keV] : 40.7607 ( -16.8275 25.9351 )
Norm@50keV : 3.14996E-03 ( -0.00314993 0.0138778 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.66 using 59 bins.
Reduced chi-squared = 1.0475
# Null hypothesis probability of 3.78e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 125.7 sec: 0.101048 ( -0.0129115 0.012997 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.30861e-07 ( -1.22383e-07 1.39672e-07 ) ergs/cm2
Band function
Time interval is from 7.832 sec. to 133.496 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.0155 (-1.33465 1.51543)
R^2/D10^2 : 4.97372E-02 (-0.0206514 0.035868)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.62e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.278e-07 2.521e-08
25- 50 3.184e-07 5.204e-08
50-150 1.669e-07 5.181e-08
15-150 6.132e-07 1.076e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 63.9657 (-19.3664 34.1058)
Norm : 0.537441 (-0.0964982 0.116469)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.98e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.714e-07 2.809e-08
25- 50 2.659e-07 3.878e-08
50-150 3.187e-07 1.094e-07
15-150 7.561e-07 1.448e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.70831 (-2.0651 2.49858)
R1^2/D10^2 : 0.473258 (-0.361366 6.00119)
kT2 [keV] : 14.0996 (-3.16075 6.54859)
R2^2/D10^2 : 1.04671E-02 (-0.00862896 0.0209053)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.70e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.682e-07 9.088e-08
25- 50 2.703e-07 1.390e-07
50-150 2.736e-07 1.618e-07
15-150 7.121e-07 3.725e-07
Peak spectrum fit
Power-law model
Time interval is from 65.004 sec. to 66.004 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.80496 ( -0.7206 0.83637 )
Norm@50keV : 2.69233E-03 ( -0.00128861 0.00115014 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.94 using 59 bins.
Reduced chi-squared = 0.911228
# Null hypothesis probability of 6.65e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.371733 ( -0.136076 0.136146 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.47851e-08 ( -1.09067e-08 1.16131e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 65.004 sec. to 66.004 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.16325 ( -2.26183 4.51821 )
Epeak [keV] : 64.2172 ( -9999.26 -9999.27 )
Norm@50keV : 1.71110E-03 ( -0.00170807 0.0426816 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.73 using 59 bins.
Reduced chi-squared = 0.92375
# Null hypothesis probability of 6.37e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.372475 ( -0.137222 0.135788 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.95839e-08 ( -1.33234e-08 1.1582e-08 ) ergs/cm2
Band function
Time interval is from 65.004 sec. to 66.004 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.3615 (-5.15324 13.5975)
R^2/D10^2 : 0.143441 (-0.136654 1.80242)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.14e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.171e-09 2.045e-09
25- 50 8.284e-09 5.230e-09
50-150 4.787e-09 3.698e-09
15-150 1.624e-08 1.086e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.9478 (-99.9975 -99.9975)
Norm : 1.62965 (-0.689104 1.45398)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.48e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.260e-09 2.748e-09
25- 50 7.365e-09 4.649e-09
50-150 1.193e-08 9.860e-09
15-150 2.356e-08 1.697e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.34028 (-2.48546 6.42304)
R1^2/D10^2 : 3.44542 (-3.32982 372.218)
kT2 [keV] : 24.5117 (-14.1925 -24.533)
R2^2/D10^2 : 5.70253E-03 (-0.00559648 0.120224)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.05e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.192e-09 3.043e-09
25- 50 5.457e-09 2.925e-09
50-150 1.513e-08 1.121e-08
15-150 2.578e-08 1.326e-08
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.76321 ( -0.193608 0.201165 )
Norm@50keV : 1.13435E-03 ( -0.000151205 0.000148558 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.02e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 64.87 sec: 0.154137 ( -0.0176194 0.0176232 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.78521e-07 ( -9.21757e-08 9.40712e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.764809 ( -1.06876 0.865296 )
Epeak [keV] : 52.5720 ( -11.3758 62.9369 )
Norm@50keV : 4.22492E-03 ( -0.00422492 0.0130412 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.15e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 64.87 sec: 0.149270 ( -0.018035 0.018082 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.14725e-07 ( -9.82761e-08 1.06337e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.44e-07
S(50-100 keV) = 2.46e-07
T90 vs. Hardness ratio plot
T90 = 114.304000020027 sec.
Hardness ratio (energy fluence ratio) = 1.0082
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.07924
Count Ratio (50-100 keV) / (15-25 keV) = 0.48154
Mask shadow pattern
IMX = 6.251576326169320E-02, IMY = 5.267702996374011E-02
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
Spacecraft aspect plot
Bright source in the pre-burst/pre-slew/post-slew images
Pre-burst image of 15-350 keV band
Time interval of the image:
-239.000000 7.832000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6501 22.0317 1.7 43.9 49.3 8.7820 6.9 1.4 Crab
135.5086 -40.5354 1.4 36.8 -152.0 3.9398 8.0 1.5 Vela X-1
148.3825 1.1164 2.5 50.1 145.8 8.6057 4.6 ------ UNKNOWN
79.3905 -14.3963 2.8 21.5 -9.6 1.5818 4.1 ------ UNKNOWN
98.8866 -29.0207 2.5 11.0 -94.9 1.6449 4.6 ------ UNKNOWN
41.6138 -15.9787 2.2 57.0 -24.2 9.0041 5.2 ------ UNKNOWN
135.8459 -59.4945 2.9 48.1 -129.3 6.5406 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
7.832000 72.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6122 22.1306 5.4 44.0 49.3 -0.8009 -2.2 7.1 Crab
135.4844 -40.6028 4.5 36.8 -151.9 -0.3447 -2.6 3.5 Vela X-1
96.8670 -20.0414 0.9 4.7 -40.1 1.2493 12.3 ------ UNKNOWN
50.8830 -12.4634 2.5 48.9 -17.4 1.1118 4.7 ------ UNKNOWN
52.0145 -17.3845 2.4 46.9 -23.7 0.9834 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
111.100600 963.120000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5272 -40.5198 1.8 38.8 -147.3 11.5471 6.4 2.1 Vela X-1
94.0632 11.9191 4.6 32.1 77.0 6.2389 2.5 ------ UNKNOWN
117.1077 1.4607 2.9 29.3 127.3 7.1407 4.0 ------ UNKNOWN
48.4575 -19.2034 3.2 45.4 -15.5 7.1337 3.6 ------ UNKNOWN
140.2708 -55.6603 3.1 48.1 -129.3 19.5314 3.7 ------ UNKNOWN
Plot creation:
Sat Mar 9 15:17:55 EST 2024